Physics Flashcards
1mCi=
37 MBq
Auger effect
When electron drops a level to fill a sudden vacancy energy is not emitted but transmitted to another electron ejecting it too - AUGER ELECTRON
Characteristic X-rays
Occur when an inner shell electron is ejected and its vacancy is filled by another electron
Curie (Ci)
Radioactivity - disintegrations per second 1mCi=37MBq
Roentgen
Radioactivity exposure - radiation in environment
Gray (Gy)
Radiation dose
1 Gy=100 RAD
(Radiation Absorbed Dose)
REM
Radiation absorbed by tissue
(Radiation Equvalent Man)
100 RAD=100 REM=1 Sv
Z
Atomic number (# protons)
A
Atomic mass
201Tl energy emssion
80 keV mercury X-rays
99mTc energy emission
140 keV gamma
17 segment model
Recombination zone
in gas-filled detector
unusable – higher probability of recombination of ion pairs than their detection
Geiger-Mueller counter
* output independent of absorbed energy
* used for survey meters
* 10x more sensitive than ion chamber
NaI scintillator
- dense – good absorber of gamma-rays
- efficient scintillator – 30 photons/keV
- light output proportional to amount radiation absorbed
- very fragile
Gamma camera energy resolution at 140 keV
9-11%
FWHM
Full width at half maximum – curve spread at the location 50% down on each side from peak amplitude
Collimator
Septa between holes absorb photons travelling in oblique lines so they never strike the detector
Gamma-camera ENERGY correction
- Decreases the system’s FWHM
- improves contrast (ability to resolve 2 points in space)
Gamma-camera LINEARITY correction
- PMT has a non-linear response to light across its face
- increased sensitivity at edges compared to center
- consequently, events at edges are misposition toward the center of the PMT
Gamma-camera UNIFORMITY correction
- aquire a high-count flood
- measure the average counts per pixel
- for each pixel compute a correction factor
- store corrections as a uniformity correction map
- correct clinical studies by multiplying each pixel in the image by its corresponding factor from the map
Parallel-hole collimator response to radiation
Collimator specs
1) energy (keV);
* thinkness of septa and materials used*
2) spacial resolution
* FWHM of 1 mm pint source @ 10 cm away*
3) sensitivity
* CPS/mCi (counts/second/radiation)*
Parallel-hole collimator design
System resolution
Rs2=Rc2 + Ri2
Rc (collimator) ~ 8 mm
Ri (instrinsic) ~ 3 mm
Rs (system) ~ 8.5 mm
Effect of source to collimator distance
Degrades resolution but not sensitivity
Non-standard collimators
New design collimators
Angular sampling
How many projections
(recommended # is 64)
Star artifact
Filtered backprojection
Mathematical filter to remove star artifact
(RAMP FILTER)
Point response function
RAMP artifact
FREQUENCY DISTRIBUTION
in SPECT imaging
low frequency = gross objects
mid frequency = detail + noise
high frequency = noise + detail
Effect of UNDERFILTERING
- can create lesions
- cut-off frequency set too high
Effect of OVERFILTERING
- can mask a lesion
- cut-off frequency set too low
ISOBARS
isobar – equal “a” nucleons
9943Tc and 9942Mo
ISOTOPES
Isotopes - Equal Protons (z)
ISOTONES
Isotones - Equal neutrons (a - z)
ISOMERS
Isomers – same radionuclide, but different energy state
99mTc (metastable) and 99Tc
BETA- emission
BETA+ emission
ELECTRON CAPTURE
admissible 99Mo breakthrough
<0.15 uCi/1 mCi Tc (at time of dose administration)
Aluminum +++
admissible impurity level
<10 PPM
admissible HRTC (hydrolyzed reduced Technetium)
<2%